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<div class="">Dear CEDAR Community,</div>
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We are now soliciting abstract submissions to the<b class="">:<br class="">
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<b class="">Royal Astronomical Society’s <span data-markjs="true" class="marksxhvucu72" data-ogac="" data-ogab="" data-ogsc="" data-ogsb="">Specialist</span> <span data-markjs="true" class="marklvgxu2h4j" data-ogac="" data-ogab="" data-ogsc="" data-ogsb="">Discussion</span> Meeting</b> on <b class="">Global
Monitoring of Geospace</b></div>
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<div style="text-align: justify; margin: 0px;" class=""><b class="">Date, time: 14th January 2022, tentatively from 10:30 – 15:30 UT. </b></div>
<div style="text-align: justify; margin: 0px;" class=""><b class="">Format: TBC, possibly a hybrid meeting between the Royal Astronomical Society, London, UK and online </b></div>
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<div style="text-align: justify; margin: 0px;" class=""><span style="color: rgb(32, 33, 36); font-size: 14px; font-family: Roboto, Arial, sans-serif; font-weight: bold; background-color: white; letter-spacing: 0.20000000298023224px;" class="">Abstract deadline:
26th November 2021</span></div>
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<div class=""><b class=""><span style="letter-spacing: 0.20000000298023224px;" class="">What is this meeting about?</span><span style="letter-spacing: 0.20000000298023224px;" class=""> </span></b>
<div class="">The interaction between the solar wind and the Earth’s magnetosphere, and the geospace dynamics that result, comprise a fundamental aspect of heliophysics. Understanding how this vast system works requires knowledge of energy and mass transport,
and a comprehension of coupling between regions and between plasma and neutral populations. Missions such as Cluster, THEMIS, Swarm, and Magnetospheric Multi-Scale, like their predecessors, explore the magnetosphere in situ, making incredibly precise local
measurements of the plasma processes that drive the behaviour of the magnetosphere on the microscale, and that enable transport and coupling. However, we are still unable to quantify the global effects of those drivers, including the conditions that prevail
throughout geospace, and how they evolve. This information is the key missing link for developing a complete understanding of how the Sun gives rise to and controls the Earth’s plasma environment.</div>
<div class="">A global perspective can be provided by remote imaging, e.g. in IR, visible, FUV and X-ray, including images of aurorae, EUV images of the plasmasphere, ENA images of the ring current and soon soft X-ray images of the Earth's magnetosheath and
cusps with the SMILE mission. The aim of this <span data-markjs="true" class="marksxhvucu72" data-ogac="" data-ogab="" data-ogsc="" data-ogsb="">Specialist</span> <span data-markjs="true" class="marklvgxu2h4j" data-ogac="" data-ogab="" data-ogsc="" data-ogsb="">Discussion</span> Meeting
is to review the remote sensing techniques and observations which provide the global view necessary for a joined-up approach to understanding the details of the interactions, and to validate the many global models which have been developed to describe them.
This meeting is targeted at the heliospheric, magnetospheric and space plasma scientific communities; it will be a forum for <span data-markjs="true" class="marklvgxu2h4j" data-ogac="" data-ogab="" data-ogsc="" data-ogsb="">discussion</span>s reflecting on
the results achieved so far, considering their implications and looking forward to forthcoming missions and observing opportunities, of which these communities will be the main users and beneficiaries.</div>
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<b class="">To submit your abstract, please either:</b></div>
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<li class=""><b class="">Fill in the following form: <a href="https://eur02.safelinks.protection.outlook.com/?url=https%3A%2F%2Fdocs.google.com%2Fforms%2Fd%2Fe%2F1FAIpQLSdieY9SryO4e2NrOocY2yIvfJz2P7OCxQKvGLQ_gwP-CTs_Zg%2Fviewform&data=04%7C01%7Cwalach%40live.lancs.ac.uk%7Ca7ea6312e89646d86b8a08d9aa63f78c%7C9c9bcd11977a4e9ca9a0bc734090164a%7C0%7C0%7C637728169334044736%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C2000&sdata=BzlVOZaB8jXokt%2FmMQRRUAIPwq8RS80uSVq376v%2BV7o%3D&reserved=0" originalsrc="https://docs.google.com/forms/d/e/1FAIpQLSdieY9SryO4e2NrOocY2yIvfJz2P7OCxQKvGLQ_gwP-CTs_Zg/viewform" shash="SSO3V1gGobnXdEioqdsKQJHyhHhKueISit6NH19gPNKx8f3ZOHno0kil6DFEWBYP8K97RDuPEJ5SH8JAXlDyr6AIL1DRXh9q4L0qj5rttKG8M87uFbbUZWN6XuB3gL/cT/C5V0wfn582hs2OGi9PZf6o/1Knyyh92J1fkyH59Ck=" target="_blank" rel="noopener noreferrer" data-auth="VerificationFailed" title="" data-linkindex="0" class="">https://docs.google.com/forms/d/e/1FAIpQLSdieY9SryO4e2NrOocY2yIvfJz2P7OCxQKvGLQ_gwP-CTs_Zg/viewform</a> ; </b></li><li style="display: block;" class=""><b class=""><br class="">
</b></li><li class=""><b class="">Or if you cannot access the Google form, please email <br class="">
</b></li><li style="display: block;" class=""><b class=""><a href="mailto:m.walach@lancaster.ac.uk" class="">m.walach@lancaster.ac.uk</a></b><br class="">
</li></ol>
<div class=""><b class="">Please note that meeting registration will be required via the Royal Astronomical Society (the <span data-markjs="true" class="mark84cop9iso" data-ogac="" data-ogab="" data-ogsc="" data-ogsb="">meetings</span> are free to Fellows and
£5 for non-fellows). This will be separate to the abstract submission and circulated closer to the time. </b><br class="">
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Best wishes,</div>
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Maria Theresia-Walach, Michaela Mooney, Jenny Carter<br class="">
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Maria-Theresia Walach<br class="">
Senior Research Associate<br class="">
Space and Planetary Physics Group<br class="">
Physics Department<br class="">
Lancaster University<br class="">
Lancaster<br class="">
LA1 4YB<br class="">
UK</div>
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